On the radial abundance gradients of nitrogen and oxygen in the inner Galactic disc
Author:
Affiliation:
1. Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain
2. Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
Abstract
Funder
Consejo Nacional de Ciencia y Tecnología
Agencia Estatal de Investigación
Ministry of Science, Innovation and Universities
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/staa3903/35931241/staa3903.pdf
Reference85 articles.
1. Galactic Abundance Gradients from Infrared Fine‐Structure Lines in Compact HiiRegions
2. The Te[N ii]–Te[O iii] temperature relation in H ii regions and the reliability of strong-line methods
3. The Galactic radial abundance gradients of C, N, O, Ne, S, Cl, and Ar from deep spectra of H ii regions
4. Estimating Distance from Parallaxes. IV. Distances to 1.33 Billion Stars in Gaia Data Release 2
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